FoF 1394
(LP 1394)
0.17
UTI
0.0
CN
0.04
Cdens
0.75
CC3
0.03
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
1.3 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.75 High quality
- Clit 0.03 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
FoF 1394 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 103.454 | 1.601 | 0.227 | -0.541 | -0.062 | â |
| Almeida et al. | 2025 | 103.447 | 1.602 | â | â | â | â |
| He et al. | 2023 | 103.483 | 1.591 | 0.23 | -0.54 | -0.075 | â |
| Dias et al. | 2021 | 103.447 | 1.602 | 0.234 | -0.553 | -0.041 | 58.299 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.18 | 1.43 | â | 23 | -0.107 | 270 | â | â |
| Almeida et al. | 2025 | 3.18 | 1.43 | â | 23 | â | 270 | â | â |
| He et al. | 2023 | 3.80 | 1.45 | â | 50 | â | â | â | â |
| Dias et al. | 2021 | 3.18 | 1.43 | â | 23 | -0.107 | â | â | â |
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.